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http://hdl.handle.net/10261/204753
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dc.contributor.author | Rousseau-Nepton, L | - |
dc.contributor.author | Martin, R.P. | - |
dc.contributor.author | Robert, C | - |
dc.contributor.author | Drissen, L. | - |
dc.contributor.author | Amram, P | - |
dc.contributor.author | Prunet, S | - |
dc.contributor.author | Martín, T. | - |
dc.contributor.author | Moumen, I | - |
dc.contributor.author | Adamo, A | - |
dc.contributor.author | Alarie, A | - |
dc.contributor.author | Barmby, P. | - |
dc.contributor.author | Boselli, A | - |
dc.contributor.author | Bresolin, F | - |
dc.contributor.author | Bureau, M | - |
dc.contributor.author | Chemin, L. | - |
dc.contributor.author | Fernandes, RC | - |
dc.contributor.author | Combes, F. | - |
dc.contributor.author | Crowder, C | - |
dc.contributor.author | Della Bruna, L | - |
dc.contributor.author | Duarte Puertas, Salvador | - |
dc.contributor.author | Egusa, F | - |
dc.contributor.author | Epinat, B | - |
dc.contributor.author | Ksoll, VF | - |
dc.contributor.author | Girard, M | - |
dc.contributor.author | Llanos, VG | - |
dc.contributor.author | Gouliermis, D | - |
dc.contributor.author | Grasha, K | - |
dc.contributor.author | Higgs, C | - |
dc.contributor.author | Hlavacek-Larrondo, Julie | - |
dc.contributor.author | Ho, IT | - |
dc.contributor.author | Iglesias-Páramo, J. | - |
dc.contributor.author | Joncas, G | - |
dc.contributor.author | Kam, ZS | - |
dc.contributor.author | Karera, P | - |
dc.contributor.author | Kennicutt, R.C. | - |
dc.contributor.author | Klessen, RS | - |
dc.contributor.author | Lianou, S | - |
dc.contributor.author | Liu, L. | - |
dc.contributor.author | Liu, Q. | - |
dc.contributor.author | de Amorim, A.L. | - |
dc.contributor.author | Lyman, J. D. | - |
dc.contributor.author | Martel, H | - |
dc.contributor.author | Mazzilli-Ciraulo, B | - |
dc.contributor.author | McLeod, AF | - |
dc.contributor.author | Melchior, AL | - |
dc.contributor.author | Millan, I | - |
dc.contributor.author | Mollá, M. | - |
dc.contributor.author | Momose, R | - |
dc.contributor.author | Morisset, C. | - |
dc.contributor.author | Pan, HA | - |
dc.contributor.author | Pati, AK | - |
dc.contributor.author | Pellerín, A. | - |
dc.contributor.author | Pellegrini, E | - |
dc.contributor.author | Pérez, I. | - |
dc.contributor.author | Petric, A | - |
dc.contributor.author | Plana, H | - |
dc.contributor.author | Rahner, D | - |
dc.contributor.author | Lara, TR | - |
dc.contributor.author | Sanchez-Menguiano, L | - |
dc.contributor.author | Spekkens, K | - |
dc.contributor.author | Stasinska, G | - |
dc.contributor.author | Takamiya, M | - |
dc.contributor.author | Asari, N.V. | - |
dc.contributor.author | Vílchez Medina, José Manuel | - |
dc.date.accessioned | 2020-03-23T09:12:30Z | - |
dc.date.available | 2020-03-23T09:12:30Z | - |
dc.date.issued | 2019 | - |
dc.identifier | doi: 10.1093/mnras/stz2455 | - |
dc.identifier | issn: 0035-8711 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society 489(4): 5530- 5546 (2019) | - |
dc.identifier.uri | http://hdl.handle.net/10261/204753 | - |
dc.description.abstract | SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing programme designed to investigate massive star formation and HII regions in a sample of local extended galaxies. The programme will use the imaging Fourier transform spectrograph SITELLE at the Canada-France-Hawaii Telescope. Over 355 h (54.7 nights) have been allocated beginning in fall 2018 for eight consecutive semesters. Once completed, SIGNALS will provide a statistically reliable laboratory to investigate massive star formation, including over 50 000 resolved HII regions: the largest, most complete, and homogeneous data base of spectroscopically and spatially resolved extragalactic HII regions ever assembled. For each field observed, three datacubes covering the spectral bands of the filters SN1 (363386 nm), SN2 (482-513 nm), and SN3 (647-685 nm) are gathered. The spectral resolution selected for each spectral band is 1000, 1000, and 5000, respectively. As defined, the project sample will facilitate the study of small-scale nebular physics and many other phenomena linked to star formation at a mean spatial resolution of similar to 20 pc. This survey also has considerable legacy value for additional topics, including planetary nebulae, diffuse ionized gas, and supernova remnants. The purpose of this paper is to present a general outlook of the survey, notably the observing strategy, galaxy sample, and science requirements.© 2019 The Author(s).Published by Oxford University Press on behalf of the Royal Astronomical Society | - |
dc.description.sponsorship | This research was based on observations obtained at the CFHT, which is operated from the summit of Mauna Kea by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. The authors wish to recognize and acknowledge the very significant cultural role that the summit of Mauna Kea has always had within the indigenous Hawaiian community. The authors are most grateful to have the opportunity to conduct observations from this mountain. The observations were obtained with SITELLE, a joint project between Universite Laval, ABB-Bomem, Universite deMontreal, and the CFHT, with funding support from the Canada Foundation for Innovation (CFI), the National Sciences and Engineering Research Council of Canada (NSERC), Fonds de Recherche du Quebec -Nature et Technologies (FRQNT), and CFHT. The collaboration is grateful to the FRQNT, CFHT, the Canada Research Chair programme, the NSERC, the Swedish Research Council (Vetenskapsradet), the Swedish National Space Board (SNSB), the Royal Society and the Newton Fund via the award of a Royal Society-Newton Advanced Fellowship (NAF\R1\180403), FAPESC, CNPq, FAPESP (2014/11156-4), FAPESB (7916/2015), and CONACyT (CB2015-254132). | - |
dc.language | eng | - |
dc.publisher | Oxford University Press | - |
dc.relation.isversionof | Publisher's version | - |
dc.rights | openAccess | - |
dc.subject | surveys | - |
dc.subject | HII regions | - |
dc.subject | Galaxies: star formation | - |
dc.title | SIGNALS: I. Survey description | - |
dc.type | artículo | - |
dc.identifier.doi | 10.1093/mnras/stz2455 | - |
dc.relation.publisherversion | http://dx.doi.org/10.1093/mnras/stz2455 | - |
dc.date.updated | 2020-03-23T09:12:30Z | - |
dc.contributor.funder | Canada Foundation for Innovation | - |
dc.contributor.funder | National Research Council of Canada | - |
dc.contributor.funder | Fonds de la Recherche en Sante du Québec | - |
dc.contributor.funder | Newton Fund | - |
dc.relation.csic | Sí | - |
dc.identifier.funder | http://dx.doi.org/10.13039/501100000156 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100000046 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100001805 | es_ES |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.openairetype | artículo | - |
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IAA_2019stz2455.pdf | 12,62 MB | Adobe PDF | Visualizar/Abrir |
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